THE ORIGIN AND FATE OF THE UNIVERSE. The Scale of the Universe The solar system (see illustration)

Slides:



Advertisements
Similar presentations
LECTURE 27, DECEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Advertisements

Objectives: 1.Explain current theories of how galaxies form, and change over time. 2.Know the characteristics of the milky way galaxy. 3.Compare and contrast.
An AP strategy for analyzing poetry. TPCASTT TITLE- first impression PARAPHRASE - poem in your own words CONNOTATION – figurative language ATTITUDE –
When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
Most evidence today indicates that the age of the Universe is
Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance.
Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe.
Galaxies and the Universe
GENS X1Galaxies1 Lecture 5: Galaxies Dr Michael Burton.
GENS S1 and S2Galaxies1 Dr Michael Burton. GENS S1 and S2Galaxies2 The Structure of our Galaxy How did we find out? Herschel’s 18 th Century.
Types of Galaxies Elliptical: Spiral: Irregular:.
LECTURE 22, NOVEMBER 18, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Chapter 31 Galaxies & the Universe Review & Recap It does this by precisely measuring the speed of gas and stars around a black hole. This provides clues.
By Jaedyn Waggoner. Block C. Mr. Horton. Science 9 THE UNIVERSE.
Fire and Ice Some say the world will end in fire, Some say in ice. From what I've tasted of desire I hold with those who favor fire. But if it had to perish.
The Milky Way and Other Galaxies. Recap Canvas homework: due on Wednesday Lab this week: Galaxy Morphology Campus Observatory Milky Way galaxy –Stars:
Cosmology. Some important questions Did the universe have a beginning or has it always existed? Will the universe end? If it ends, what will happen at.
Star Systems and Galaxies Galaxies and the Big Bang Theory.
The Big Stuff Galaxies The Universe and The Big Bang.
Star Systems and Galaxies Multiple Star Systems Binary stars – star systems with two stars Eclipsing binary – system where one star periodically blocks.
GALAXIES These are galaxy clusters and separate galaxies taken by long-range telescope. The area of the sky covered is less than the diameter of the moon.
The Big Bang Hubble's Law Galaxies
Cosmology: The Study of the Universe as a Whole Physics 360 Geol 360 Astronomy John Swez.
Galaxies and the UNIVERSE.
Galaxies and the Universe
1 Galaxies The Andromeda Galaxy - nearest galaxy similar to our own. Only 2 million light years away! Galaxies are clouds of millions to hundreds of billions.
Key Topics Astronomy Unit. Big Bang Theory Big Bang Theory: most widely accepted theory for the origin of our universe billion States that
Astronomy Topic 4 Revision Booster. Milky way facts 200 billion stars 250 million years to orbit One of a group of about 30 galaxies (The local group)
Classifying galaxies Big Bang Active galaxies Our Local Group Random $ 200 $ 200$200 $ 200 $400 $ 400$400 $ 400 $600 $ 600$600 $ 600 $ 600 $800 $
Chapter 16 The Milky Way Galaxy 16.1 Overview n How many stars are in the Milky Way? – About 200 billion n How many galaxies are there? – billions.
The Nature of Galaxies Chapter 17. Other Galaxies External to Milky Way –established by Edwin Hubble –used Cepheid variables to measure distance M31 (Andromeda.
Cosmology Olber’s Paradox Big Bang Development of the Universe.
IB Physics Power Points
The Tully-Fisher Relation A relation between the rotation speed of a spiral galaxy and its luminosity The more mass a galaxy has  the brighter it is 
Complete History of the Universe (Abridged) Thursday, March 6.
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
Our Galaxy  Write you address:  Spring Cypress Road  Cypress TX,  United States of America  Earth, Solar System  2/3 Orion-Cygnus.
Do Now Put the following in order from largest to smallest Galaxy Earth’s Moon Sun Universe Planet (Earth) Solar system What is the name of our Galaxy?
“OUR GALAXY” Definition of a Galaxy: a huge group of individual stars, star clusters, dust, and gas bound together by gravity.
Quiz #10 What would really happen to you if you were to fall all the way into the Event Horizon of a black hole? We know the gravity is unbelievably strong.
Galaxies and the Universe Ch 25 Section 3. What are the objects in the sky? GALAXIES! Groups of stars, dust, and gases held together by gravity.
25-4: Galaxies Use the following PowerPoint to take notes on the final section of the chapter. Upon completion work with your partner to answer the Self.
Fate of the Universe 1)Fate of the Universe 2)Shape of the Universe 3)Large Scale Structure November 25, 2002 Final Exam will be held in Ruby Diamond Auditorium.
Star Systems & Galaxies
Dark “Dark” Energy R DARK G. Cosmology is the study of the Universe's 1. Shape.
The Shape and Fate of the Universe Assumptions in cosmology Olber’s paradox Expansion of the Universe Curvature of the Universe Fate of the Universe.
Milky Way Galaxy. Galaxy A group of stars, dust and gases held together by gravity. 170 billion galaxies in the universe 200 billion stars in a galaxy.
Chapter 20 Cosmology. Hubble Ultra Deep Field Galaxies and Cosmology A galaxy’s age, its distance, and the age of the universe are all closely related.
GALAXIES & BEYOND. What is a galaxy? A galaxy is a very large group of stars held together by gravity. Size: 100,000 ly+ Contain Billions of stars separated.
COSMOLOGY The study of the origin, structure, and future of the universe.
Galactic Jeopardy Vocabulary Galaxies Shapes of Galaxies Star Clusters Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final Jeopardy.
Aim: How did the universe form?
How fast would a galaxy 2,000 megaparsecs away be moving with respect to us, according to Hubble’s Law? Hint: H0 = 70 km/s/Mpc 1,400 km/s 14,000 km/s 140,000.
© 2017 Pearson Education, Inc.
Earth in Our Universe.
The Big Bang Evidence of creation and expansion of the Universe through Background Radiation and Investigating Spectra (color)
Galaxies and Stars Galaxies – billions of star groups
The Milky Way, Deep Space, and Beyond!
GALAXIES OF STARS & OUR UNIVERSE
GALAXIES OF STARS & OUR UNIVERSE
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
Ch. 31 – Galaxies & the Universe
The Universe Chapter 25.3.
ASTR 1040 Accel Astro: Stars & Galaxies
Do Now Put the following in order from largest to smallest Galaxy
The Components and Origin of the Universe
Galaxies.
Essential Question: What is a galaxy and how are they classified?
Lesson 5 Splash galaxy Milky Way spectrum expansion redshift big bang
The Big Bang Timeline Rapid Expansion of the Universe
Presentation transcript:

THE ORIGIN AND FATE OF THE UNIVERSE

The Scale of the Universe The solar system (see illustration)

The Scale of the Universe Nearby Star systems (see illustration)

The Scale of the Universe Galaxies –spiral galaxies (the Milky Way and the Andromeda galaxies) the arms the central bulge the halo and globular clusters

The Scale of the Universe (cont.) Galaxies –irregular galaxies –elliptical galaxies

Large Magellinic Cloud, irregular galaxy M84 Elliptical Galaxy

The Scale of the Universe (cont.) The Local Cluster or Group (see illustration)

The Scale of the Universe (cont.) Super clusters (see illustration)

The Scale of the Universe (cont.) The Universe (see illustration)

Newton’s Model Infinite and static Olber’s paradox

Evidence of Expansion Hubble’s law –doppler shift –recession velocity Vs. distance

Evidence of Expansion Background radiation –doppler shift

The Creation of the Universe The big bang –time line s s s s s s 2 s 3 minutes 300, 000 years

The Creation of the Universe The big bang –the laws of physics –where –when

The Fate of the Universe Critical mass / density

The Fate of the Universe Curvature of space –open (saddle or negative curvature) –critical (flat or no curvature) –closed (spherical or positive curvature)

Some say the world will end in fire. Some say ice. From what I’ve tasted of desire I hold with those who favor fire. But if I had to perish twice I think I know enough of hate To say that for destruction ice Is also great And would suffice.